This post is based upon my reading of the section on Quasi-Linear Equation in Arnold’s ODE.

In the previous 2 posts, we looked at linear homogeneous PDE’s:

a_1(x) \frac{\partial u}{\partial x_1} + ... + a_n(x) \frac{\partial u}{\partial x_n} = 0 (*)

The characteristic vector field corresponding to (*) is given by:

\dot{x} = (a_1, ..., a_n)

This vector field lives in the x-space. Geometrically, the restriction of any solution u(x) to a phase curve of the characteristic vector field is a constant. This is equivalent to saying that the vertical projection of the level lines of the graph of u(x) in the (x, u)-space onto the x-space gives us the phase curves of the characteristic vector field.

We also looked at linear inhomogeneous PDE’s:

a_1(x) \frac{\partial u}{\partial x_1} + ... + a_n(x) \frac{\partial u}{\partial x_n} = b(x)

Key: the characteristic vector field no longer lives in the x-space; rather, it lives inside the (x, u)-space, i.e. the space of 0-jets.

The characteristic vector field is given by:

(\dot{x}, \dot{u}) = (a_1, ..., a_n, b)

Geometrically, this means that a point x leaves point x_0 in the x-space with velocity (a_1(x_0), ..., a_n(x_0)) (i.e. a particle is moving along a phase flow of the field \dot{x} = (a_1, ..., a_n)), then the value of u(x) begins to change with velocity b(x_0).

Notice: this vector field is invariant under translation along the u-axis. Hence, the vector field is the same for any fixed u-value. The vertical projection of such vector field onto the x-space is well-defined and gives us the vector field (a_1, ..., a_n) that corresponds too the linear homogeneous PDE a_1(x) \frac{\partial u}{\partial x_1} + ... + a_n \frac{\partial u}{\partial x_n} = 0.

Quasi-linear Equation

Now, let’s look at the case where the corresponding vector field not only depends on the x-value but also the u-value, i.e.

a_1(x, u) \frac{\partial u}{\partial x_1} + ... + a_n(x, u) \frac{\partial u}{\partial x_n} = b(x, u) (**)

We can see that the linear inhomogeneous equation is really just a special case of this. The characteristic vector field for (**) is:

(\dot{x}, \dot{u}) = (a_1(x, u), ..., a_n(x, u), b(x, u))

and it lives in the (x, u)-space. But in this case, the vector field is no longer invariant under translation along the u-axis. However, the same geometric interpretation still applies.

Example: the motion of one-dimensional medium of particles moving along a line by inertia (velocity of each particle is constant) can be described by a quasi-linear equation.

Let the velocity of the particle at point x at time t be u(t, x).

Set x = \phi(t) to be the motion of a particle. Then,

\dot{x} = \dot{\phi} = u(t, \phi(t)) and

\ddot{x} = \ddot{\phi} = \frac{d}{dt} u(t, \phi(t)) = \begin{bmatrix} \frac{\partial u}{\partial t} \\ \frac{\partial u}{\partial x} \end{bmatrix} \cdot \begin{bmatrix} \dot{t} \\ \dot{\phi} \end{bmatrix} = \frac{\partial u}{\partial t} + \frac{\partial u}{\partial x} \dot{\phi}

Since the acceleration of the particle is 0, it follows that:

\frac{\partial u}{\partial t} + \frac{\partial u}{\partial x} \dot{\phi} = 0

This is the quasi-linear equation that describes the motion of the particles.

Example 1.a: Construct the graph of the solution at the instant t if u = arctan(x) for t = 0.

Key: the restriction of the characteristic vector field to the (x, u)-plane is

\dot{x} = u

\dot{u} = 0

Why? Because \dot{x} is the velocity of the particle, which by definition is u; \dot{u} is the acceleration of the particle, which we know to be zero.

The phase flows of this vector field on the (x, u)-plane is:

\phi: \tau \mapsto (x + u \tau, u)

Notice that the family of all phase flows for a fixed time \tau = \tau_0 corresponds to a diffeomorphism of the plane, more specifically, a diffeomorphism of the vector field on the plane.

Geometrically, this diffeomorphism \Psi_{\tau}: (x, u) \mapsto ( x + u \tau, u) maps the graph of the solution at the instant 0 to the graph of the solution at the instant \tau.

Given the initial point (x_0, arctan(x_0)), the corresponding point after moving along the phase flow for time \tau is (x_0 + arctan(x_0)\tau, arctan(x_0)).

Thus, for t = \tau, the graph is given by the set:

\{ (x_0 + \arctan(x_0) \tau, arctan(x_0)) : x_0 \in \mathbb{R} \}

Notice: for t \geq \pi/2, no smooth solution exists.

Example 1.b: Construct the equation for the evolution of the velocity field of a medium of noninteracting particles in a force field with force F(x) at the point x.

Let u(t, x) be the velocity of a particle at time t and position x. Let \phi(t) = x be the motion of the particle. Then,

\dot{x} = \dot{\phi}(t) = u(t, \phi(t)) and

\ddot{x} = F(\phi(t)) (the force F(x) gives us an acceleration F(x), if we assume the particle to have unit mass)

We also know that \ddot{x} = \frac{\partial u}{\partial t} + u \frac{\partial u}{\partial x}.

Thus, we obtain the equation \frac{\partial u}{\partial t} + u \frac{\partial u}{\partial x} = F(x).

Example 1.c: Solve this equation with the initial condition u|_{t=0} = 0 for the force field F(x) = -x.

Key: we focus on the restriction of the vector field to the (x, u)-plane for a fixed instant of time.

The corresponding vector field is given by:

\dot{x} = u

\dot{u} = -x (because the acceleration is F(x) = -x)

The corresponding phase curves are circles centred at the origin.

The phase flow passing through an arbitrary point (x_0, u_0) is given by \phi: \tau \mapsto (-cos(\tau) x_0, sin(\tau) u_0).

As given, the graph of the solution at the instant t = 0 is the line u = 0. The corresponding graph of the solution at t = \tau is obtained by moving each point on u = 0 along the phase flow for time \tau. In this case, this would be rotating the line u = 0 by an angle \tau clockwise. The resulting graph is on the (x, u)-plane is u(t, x) = -x tan(\tau).

Hence, the corresponding solution in the (t, x, u)-space is:

u(t, x) = -x tan(t)

Note: such a solution is well-defined on |t| < \pi /2 but not only the entire t-axis.

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